Mathematics
Scientific paper
Mar 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985mnras.213..365m&link_type=abstract
Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 213, March 15, 1985, p. 365-380.
Mathematics
7
Galactic Clusters, Galactic Structure, Partitions (Mathematics), Taxonomy, Classifying, Red Shift, Trees (Mathematics)
Scientific paper
The structure of the Hercules and Perseus superclusters has been analysed by the non-hierarchical-descendent taxonomical method. In the case of Hercules, well-defined groups are present. The membership of the galaxies with respect to the groups is given, as well as the physical parameters for the groups. A morphological type-redshift effect is present. For Perseus, the internal structure is much less well defined, as it appears as a filamentary aggregate without a clear subgrouping. Tentatively some apparent groups in it are noted and its physical parameters calculated.
Del Olmo Ascension
Moles Mariano
Perea Jaime
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